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Dynamics of Magnetized Black Holes in Anisotropic Matter Fields

Munisa BoltatoshovaInstitute of Theoretical Physics, National University of Uzbekistan, Tashkent 100174, UzbekistanBakhtiyor NarzilloevInstitute for Advanced Studies, New Uzbekistan University, Movarounnahr str. 1, Tashkent 100000, UzbekistanAhmadjon AbdujabbarovSchool of Physics, Harbin Institute of Technology, Harbin 150001, People’s Republic of ChinaBobomurat Ahmedov{Institute of Theoretical Physics, National University of Uzbekistan, Tashkent 100174, Uzbekistan

Turanian Journaljournal2025

ABI

Annotatsiya

We study the dynamics of charged test particles around magnetized black holes with anisotropic matter fields. Using the Cho–Kim solution, we analyze the effects of the anisotropy parameter K, the state parameter ω, and an external magnetic field on the effective potential, orbital stability, and the innermost stable circular orbit (ISCO). Our results show that anisotropy shifts the ISCO outward, while magnetic coupling permits stable orbits closer to the event horizon. The combined influence of anisotropy and magnetization reproduces Kerr-like orbital behavior, suggesting that such black hole configurations may act as Kerr mimickers with potentially observable astrophysical signatures.

Mavzular

Astrophysical Phenomena and Observations Pulsars and Gravitational Waves Research Astrophysics and Cosmic Phenomena

Identifikatorlar

DOI: 10.65910/turanianj.010402

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